In Problem 1.16 you calculated the pressure of the earth’s atmosphere as a function of altitude, assuming constant temperature. Ordinarily, however, the temperature of the bottommost 10-15 km of the atmosphere (called the troposphere) decreases with increasing altitude, due to heating from the ground (which is warmed by sunlight). If the temperature gradient |dT/dz|exceeds a certain critical value, convection will occur: Warm, low-density air will rise, while cool, high-density air sinks. The decrease of pressure with altitude causes a rising air mass to expand adiabatically and thus to cool. The condition for convection to occur is that the rising air mass must remain warmer than the surrounding air despite this adiabatic cooling.

a. Show that when an ideal gas expands adiabatically, the temperature and pressure are related by the differential equation

dTdP=2f+2TP

b. Assume that dT/dzis just at the critical value for convection to begin so that the vertical forces on a convecting air mass are always approximately in balance. Use the result of Problem 1.16(b) to find a formula for dT/dzin this case. The result should be a constant, independent of temperature and pressure, which evaluates to approximately 10°C/km. This fundamental meteorological quantity is known as the dry adiabatic lapse rate.

Short Answer

Expert verified
  1. The required differential equation is dTdP=2f+2TP.
  2. The required expression is dTdz=2mgkf+2.

Step by step solution

01

Part a. Step 1. Given.

The pressure of the earth’s atmosphere is a function of altitude with the temperature being constant. The temperature of the bottommost 10-15 km of the atmosphere decreases with increasing altitude due to heating from the ground.

If the temperature gradientdTdz exceeds a certain critical value then convection will occur.

02

Part a. Step 2. Formula used.

For adiabatic expansion, the relation between pressure, volume, and temperature is

PVγ=const. …… (1)

And

VTf2=const. …… (2)

Here,P is the pressure of the gas,V is the volume of the gas,T is the temperature in Kelvin,γ is the adiabatic exponent, andf is the degree of freedom γ=f+22.

03

Part a. Step 3. Calculation.

Isothermal compression is so slow that the temperature of the gas doesn’t rise at all and in adiabatic compression, the process is so fast that no heat escapes from the gas during the process. Most real compression processes will be somewhere between these extremes usually closer to the adiabatic approximation.

Differentiate equation (1) on both sides,

PVγ=const.

VγdP+γVγ1PdV=0 …… (3)

Similarly, differentiate equation (2) on both sides,

Tf2dV+f2Tf21VdT=0 …… (4)

Divide equation (3) by Vγ1on both sides

VγdP+γVγ1PdVVγ1=0VγdPVγ1+γVγ1Vγ1PdV=0

VdP+γPdV=0 …… (5)

Divide equation (4) by Tf21on both sides

Tf2dV+f2Tf21VdTTf21=0Tf2dVTf21+f2Tf21Tf21VdT=0

TdV+f2VdT=0 …… (6)

Rearrange equation (5)

dP=γPdVV …… (7)

Rearrange equation (6)

dT=f2TdVV …… (8)

Divide equation (7) by equation (8)

dTdP=2fTdVV×VγPdV

dTdP=2fTγP …… (9)

Substitutef+2f forγ in equation (9)

dTdP=2f×ff+2TP

dTdP=2f+2TP.

04

Part a. Step 4. Conclusion.

Hence the required differential equation is dTdP=2f+2TP.

05

Part b. Step 1. Given.

Barometric equation is

dPdz=mgkTP …… (1)

Here,m is mass,k is Boltzmann constant,T and P is temperature, and pressure respectively.

06

Part b. Step 2. Formula.

The relation between pressure, temperature, and volume is

dTdP=2f+2TP …… (2)

Here,f is the degree of freedom,T and P are temperature and pressure respectively.

07

Part b. Step 3. Calculation.

Isothermal compression is so slow that the temperature of the gas doesn’t rise at all and in adiabatic compression, the process is so fast that no heat escapes from the gas during the process. Most real compression processes will be somewhere between these extremes usually closer to the adiabatic approximation.

Simplify equation (1)

dPP=mgkTdz …… (3)

From equation (2), it is found that

dT=2Tf+2dPP …… (4)

Substitute mgkTdzfor dPPin equation (4)

dT=2Tf+2mgkTdzdTdz=2mgkf+2

08

Part b. Step 4. Conclusion.

Hence, the required expression is dTdz=2mgkf+2.

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Most popular questions from this chapter

An ideal diatomic gas, in a cylinder with a movable piston, undergoes the rectangular cyclic process shown in the given figure.

Assume that the temperature is always such that rotational degrees of freedom are active, but vibrational modes are "frozen out." Also assume that the only type of work done on the gas is quasistatic compression-expansion work.

(a) For each of the four steps A through D, compute the work done on the gas, the heat added to the gas, and the change in the energy content of the gas. Express all answers in terms of P1,P2,V1,andV2. (Hint: Compute ΔUbefore Q, using the ideal gas law and the equipartition theorem.)

(b) Describe in words what is physically being done during each of the four steps; for example, during step A, heat is added to the gas (from an external flame or something) while the piston is held fixed.

(c) Compute the net work done on the gas, the net heat added to the gas, and the net change in the energy of the gas during the entire cycle. Are the results as you expected? Explain briefly.

Make a rough estimate of the thermal conductivity of helium at room temperature. Discuss your result, explaining why it differs from the value for air.

Heat capacities are normally positive, but there is an important class of exceptions: systems of particles held together by gravity, such as stars and star clusters.
aConsider a system of just two particles, with identical masses, orbiting in circles about their center of mass. Show that the gravitational potential energy of this system is-2times the total kinetic energy.
bThe conclusion of part aturns out to be true, at least on average, for any system of particles held together by mutual gravitational attraction:

U¯potential=2U¯kinetic

Here each Urefers to the total energy (of that type) for the entire system, averaged over some sufficiently long time period. This result is known as the virial theorem. (For a proof, see Carroll and Ostlie (1996), Section 2.4.) Suppose, then, that you add some energy to such a system and then wait for the system to equilibrate. Does the average total kinetic energy increase or decrease? Explain.

cA star can be modeled as a gas of particles that interact with each other only gravitationally. According to the equipartition theorem, the average kinetic energy of the particles in such a star should be 32KT, whereT is the average temperature. Express the total energy of a star in terms of its average temperature, and calculate the heat capacity. Note the sign.
dUse dimensional analysis to argue that a star of mass Mand radius Rshould have a total potential energy of -GM2/R, times some constant of order 1.
eEstimate the average temperature of the sun, whose mass is 2×1030kgand whose radius is 7×108m. Assume, for simplicity, that the sun is made entirely of protons and electrons.

Even at low density, real gases don’t quite obey the ideal gas law. A systematic way to account for deviations from ideal behavior is the virial

expansion,

PVnRT(1+B(T)(V/n)+C(T)(V/n)2+)

where the functions B(T), C(T), and so on are called the virial coefficients. When the density of the gas is fairly low, so that the volume per mole is large, each term in the series is much smaller than the one before. In many situations, it’s sufficient to omit the third term and concentrate on the second, whose coefficient B(T)is called the second virial coefficient (the first coefficient is 1). Here are some measured values of the second virial coefficient for nitrogen (N2):

T(K)
B(cm3/mol)
100–160
200–35
300–4.2
4009.0
50016.9
60021.3
  1. For each temperature in the table, compute the second term in the virial equation, B(T)/(V/n), for nitrogen at atmospheric pressure. Discuss the validity of the ideal gas law under these conditions.
  2. Think about the forces between molecules, and explain why we might expect B(T)to be negative at low temperatures but positive at high temperatures.
  3. Any proposed relation between P, V, andT, like the ideal gas law or the virial equation, is called an equation of state. Another famous equation of state, which is qualitatively accurate even for dense fluids, is the van der Waals equation,
    (P+an2V2)(Vnb)=nRT
    where a and b are constants that depend on the type of gas. Calculate the second and third virial coefficients (Band C) for a gas obeying the van der Waals equation, in terms of aand b. (Hint: The binomial expansion says that (1+x)p1+px+12p(p1)x2, provided that |px|1. Apply this approximation to the quantity [1(nb/V)]1.)
  4. Plot a graph of the van der Waals prediction for B(T), choosing aand bso as to approximately match the data given above for nitrogen. Discuss the accuracy of the van der Waals equation over this range of conditions. (The van der Waals equation is discussed much further in Section 5.3.)

Does it ever make sense to say that one object is "twice as hot" as another? Does it matter whether one is referring to Celsius or Kelvin temperatures? Explain.

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